Image Details
Caption: Figure 4.
Velocity dispersion of [O III] vs. stellar velocity dispersion for Type 1 AGNs: [O III] fitted with a double Gaussian model (left) or a single Gaussian model (middle). The best-fit relation for Type 1 AGNs is represented by the solid line, while the dash-dotted line denotes the unity relation. The best-fit relation for Type 2 AGNs from Woo et al. (2016) is also shown (dashed line). The right panel shows the distributions of the ratio of σ[O III] to σ* for Type 1 AGNs: double Gaussian [O III] (red) and single Gaussian [O III] (blue).
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